Abstract

This study aims to investigate how accurate are TASMICS and TASMIP models in predicting the X-ray output of some Conventional Radiology X-ray units with high frequency generators. The X-ray output in microgray per milliampere seconds (μGy/mAs) at 100 cm from the X-ray tube was determined for selected high voltages and taking into account the total filtration. The X-ray output was then measured directly with the multi-purpose detectors (MPD), Raysafe X2. The maximum relative error between measured and predicted values was found to be equal to 20%. The maximum relative error between measured and predicted values obtained demonstrates the difficulty of accurately predicting the X-ray tube output using TASMICS and TASMIP models since they are based on fixed anode angles and different composition of the tungsten anode.

Highlights

  • Several computational methods are used to characterize X-ray spectra

  • The maximum relative error between measured and predicted values obtained demonstrates the difficulty of accurately predicting the X-ray tube output using TASMICS and TASMIP models since they are based on fixed anode angles and different composition of the tungsten anode

  • This work aims to evaluate the accuracy of the assessment of the Entrance Surface Exposure using TASMIP and TASMICS models and the examination parameters used in conventional radiography

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Summary

Introduction

Several computational methods are used to characterize X-ray spectra. Boone and Seibert [1] reported on a method for computing X-ray spectra based on the method of interpolating polynomials, called TASMIP, this model computes tungsten anode X-ray spectra in 1 keV energy bins between 30 and 140 kV and provides accurate spectral estimation based on the measurements of Fewell et al [2]. J.H. Hernandez and J.M. Boone [3] later developed a new method named Tungsten Anode Spectral Model using Interpolating Cubic Splines (TASMICS).

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